The $B$ Anomalies and non-SMEFT New Physics

Abstract

The modern viewpoint is that the Standard Model is the leading part of an effective field theory that obeys the symmetry $SU(3)_C \times SU(2)_L \times U(1)_Y$. Since the discovery of the Higgs boson, it is generally assumed that this symmetry is realized linearly (SMEFT), but a nonlinear realization (e.g., HEFT) is still possible. The two differ in their predictions for the size of certain low-energy dimension-6 four-fermion operators: for these, HEFT allows $O(1)$ couplings, while in SMEFT they are suppressed by a factor $v^2/\Lambda_{\rm NP}^2$, where $v$ is the Higgs vev. In this talk, I argue that (i) such non-SMEFT operators contribute to both $b \to s \ell^+ \ell^-$ and $b \to c \,\tau^- {\bar\nu}_\tau$, transitions involved in the present-day $B$ anomalies, (ii) the contributions to $b \to s \ell^+ \ell^-$ are constrained to be small, at the SMEFT level, and (iii) the contribution to $b \to c \,\tau^- {\bar\nu}_\tau$ can be sizeable. I show that the angular distribution in ${\bar B} \to D^* (\to D \pi') \, \tau^{-} (\to \pi^- \nu_\tau) {\bar\nu}_\tau$ contains enough information to extract the coefficients of all new-physics operators. The measurement of this angular distribution can tell us if non-SMEFT new physics is present.